English

Regularized phase-space volume for the three-body problem

Earth and Planetary Astrophysics 2022-12-07 v1 Statistical Mechanics High Energy Physics - Theory

Abstract

The micro-canonical phase-space volume for the three-body problem is an elementary quantity of intrinsic interest, and within the flux-based statistical theory, it sets the scale of the disintegration time. While the bare phase-volume diverges, we show that a regularized version can be defined by subtracting a reference phase-volume, which is associated with hierarchical configurations. The reference quantity, also known as a counter-term, can be chosen from a 1-parameter class. The regularized phase-volume of a given (negative) total energy, σˉ(E)\bar\sigma(E), is evaluated. First, it is reduced to a function of the masses only, which is sensitive to the choice of a regularization scheme only through an additive constant. Then, analytic integration is used to reduce the integration to a sphere, known as shape sphere. Finally, the remaining integral is evaluated numerically, and presented by a contour plot in parameter space. Regularized phase-volumes are presented for both the planar three-body system and the full 3d system. In the test mass limit, the regularized phase-volume is found to become negative, thereby signalling the breakdown of the non-hierarchical statistical theory. This work opens the road to the evaluation of σˉ(E,L)\bar\sigma(E,L), where LL is the total angular momentum, and it turn, to comparison with simulation determined disintegration times.

Keywords

Cite

@article{arxiv.2205.04294,
  title  = {Regularized phase-space volume for the three-body problem},
  author = {Yogesh Dandekar and Barak Kol and Lior Lederer and Subhajit Mazumdar},
  journal= {arXiv preprint arXiv:2205.04294},
  year   = {2022}
}

Comments

27 pages, 6 figures

R2 v1 2026-06-24T11:11:32.510Z